For the radio telescope to function properly, the surrounding areas must be free from interferers, especially at the Ku band of operation. It will be laborious to manually keep scanning the radio space for potential interferers, which is why we researched into developing a system to help with interference studies for the radio telescope project.
Conventionally, the noise parameters for a linear two-port device-under-test (DUT) are measured using a mechanical impedance tuner. The mechanical impedance tuner is used to vary the source impedance seen from the DUT. An experimental search for the minimum noise figure using the mechanical impedance tuner results in the optimum impedance too. One or several nonsingular noise figure measurements then result in the complete determination of the noise parameters. The noise parameters determined by this technique generally show fluctuation and are inaccurate. Commercial test set are ridiculously expensive. This research employs a six-port network to find alternative noise parameters measurement technique that will be fast, accurate, simple and at very low cost.
We research into design concepts, techniques for achieving good input match and excellent radiation patterns and characteristics suitable for various antenna types and for various wireless applications such as RFID, GPS, GSM and WLAN.
To build capacity for high-quality applicable and publishable research; breaking the frontiers of technology while making impacts in the scientific community.